| Start Date | Context | Status | Description |
|---|---|---|---|
| 2025-11-03 | hst_1294.pmap | latest | Delivery of new STIS CCD bias and dark reference files for CCD data taken between September 30, 2025 and October 31, 2025. The files were generated from data taken in the same time frame under STIS calibration programs 17631 and 17633. |
| 2025-10-31 | hst_1293.pmap | archived | The previous detector linearity correction file contains coefficients derived and averaged over each of the four detector quadrants. In contrast, this file contains pixel-based non-linearity correction coefficients, which significantly improves the linearity response at high fluence levels as well as the performance of the automated cosmic ray fitting procedure. Consequently, the new solution improves signal-to-noise and photometric accuracy, and should be implemented into calwf3 for the benefit of users. |
| 2025-10-30 | hst_1292.pmap | archived | The ACS WFC bias, dark, CTE dark, and sink files were generated following the ACS WFC anneal on October 22, 2025, and should be used to calibrate ACS WFC observations taken between September 23, 2025 and October 22, 2025. |
| 2025-10-30 | hst_1291.pmap | archived | These WFC3 UVIS superdarks will affect all UVIS data taken from September 19, 2025 to October 13, 2025. Currently, the automated calibration pipeline and CRDS have only WFC3 UVIS drk and dkc reference files with USEAFTER dates of up to September 16, 2025. The automated pipeline should now use these reference files to perform dark subtraction on any UVIS datasets obtained between the dates above, as they represent the most accurate picture of dark current and hot pixels for this time period. The new bad pixel table with USEAFTER of September 19, 2025 was generated using data taken from September 19, 2025, through October 16, 2025. Currently, the Calibration Reference Data System only has WFC3 UVIS bad pixel reference tables up to a USEAFTER date August 20, 2025. The automated pipeline should now use this reference file as the bad pixel table on any UVIS datasets obtained from September 19, 2025 to present because it represents the most accurate measure of pixel stability at the time of the science observation. For more details regarding both deliveries, please see the Context History and select -all contexts- on the CRDS homepage. |